Image Details
Caption: Figure 5.
M–L relations for O24_ML4h_RA models (fH = 0.02, fenv = 0.04, ηR = 0.4) with W0 = 0 (gray lines) and the highest initial rotation rate of W0 = 0.65 (blue lines), and for models of the O24_ML8h_RA set (with twice as large ηR = 0.8) and W0 = 0.65, for MW, LMC, and SMC metallicities (Z = 0.014, 0.006, and 0.002 in the left, middle, and right panels, respectively). The theoretical relations are confronted with determinations from A. Gallenne et al. (2018, 2025), B. Pilecki et al. (2018), and N. R. Evans et al. (2024).
© 2026. The Author(s). Published by the American Astronomical Society.